2015/12/31 by Hakan Cebeci, Nülifer Özdemir, Seçil Şentorun
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #Equations of motion #Jacobian matrix and determinant #Mathematical physics #Mathematics #Motion (physics) #Observable #Orbit (dynamics) #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Spacetime #Test particle #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.93.104031
published as Phys. Rev. D 93, 104031 (2016) · 42 pages, improved version, to appear in PRD
arxiv created 2016/05/09 · openalex publication_date 2016/05/16 · arxiv updated 2016/05/25 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In this work, we study the motion of charged test particles in Kerr-Newman-Taub-NUT spacetime. We analyze the angular and the radial parts of the orbit equations and examine the possible orbit types. We also investigate the spherical orbits and their stabilities. Furthermore, we obtain the analytical solutions of the equations of motion and express them in terms of Jacobian and Weierstrass elliptic functions. Finally, we discuss the observables of the bound motion and calculate the perihelion shift and Lense-Thirring effect for the bound orbits.